MSI Seminar - A natural wind tunnel for plasma astrophysics

Jonathan Squire (University of Otago)

Oct 6, 2020 3:30 PM
MSI Seminar

Title: A natural wind tunnel for plasma astrophysics: learning from in-situ observations of the solar wind

Abstract:

The dynamics of hot, diffuse plasmas underlie most high-energy phenomena, from the origin and propagation of cosmic rays to the heating of galaxy clusters. They are also rich in interesting physics, with the lack of frequent inter-particle collisions causing surprising and complex thermodynamical properties that depend in detail on how the system is stirred. In studying the basic properties of such plasmas, we have a resource unrivalled in most of the rest of astrophysics: exquisitely detailed measurements of fluctuations, particle distributions, and structures from inside the natural wind tunnel formed by our solar wind. In this talk, I will explore recent work on understanding turbulence in collisionless plasmas and how this can be studied from a mix of theory and in-situ spacecraft observations. The goal is both to better understand the basic physics of this interesting state of matter and to provide concrete models for still-uncertain astrophysical processes. As important examples, I will consider the electron-to-ion heating ratio in black-hole accretion flows and the propagation of cosmic rays through our galaxy.


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Upcoming Seminars

TSI Seminars take place weekly during the Fall and Winter terms. TSI seminars are intended to be accessible to scientists from the entire breadth of backgrounds at TSI, including, Physics, Planetary Science, Geology, Atmospheric Science, and Astrobiology. Our seminar series is partially funded by the Centre de recherche en astrophysique du Québec (CRAQ).

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